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J/MNRAS/396/2194    Radial velocity curve of V440 Per        (Baranowski+, 2009)

V440 Per: the longest-period overtone Cepheid. Baranowski R., Smolec R., Dimitrov W., Kwiatkowski T., Schwarzenberg-Czerny A., Bartczak P., Fagas M., Borczyk W., Kaminski K., Moskalik P., Ratajczak R., Rozek A. <Mon. Not. R. Astron. Soc., 396, 2194-2200 (2009)> =2009MNRAS.396.2194B
ADC_Keywords: Stars, variable ; Radial velocities Keywords: hydrodynamics - methods: data analysis - techniques: spectroscopic - stars: individual: V440 Per - stars: oscillations - Cepheids Abstract: 440 Per is a Population I Cepheid with a period of 7.57d and low-amplitude, almost sinusoidal light and radial velocity curves. With no reliable data on the first harmonic, its pulsation mode identification remained controversial. We obtained a radial velocity curve of V440 Per with our new high-precision and high-throughput Poznan Spectroscopic Telescope. Description: The PST is located in Poland at the Borowiec station, 20km south from Poznan city, at a meagre elevation of 123m above sea level. The PST consists of parallel twin 0.4-m Newton telescopes of the f ratio 4.5, fixed on a single parallactic fork mount. In total 158 radial velocity measurements of V440 Per were obtained with the PST from 2007 August 15 to 2008 July 03. Objects: --------------------------------------------- RA (2000) DE Designation(s) --------------------------------------------- 02 23 51.7 +55 21 53 V440 Per = HD 14662 --------------------------------------------- File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table1.dat 24 158 Poznan Spectroscopic Telescope (PST) radial velocities of V440 Per
Byte-by-byte Description of file: table1.dat
Bytes Format Units Label Explanations
1- 10 F10.4 d MJD Modified Julian date 13- 17 F5.2 km/s DRV Differential radial velocity, zero shifted by about -26.3±0.2km/s 20- 24 F5.2 km/s DRVc Differential radial velocity, corrected for instrumental effects (see text)
History: From electronic version of the journal
(End) Patricia Vannier [CDS] 02-Nov-2009
The document above follows the rules of the Standard Description for Astronomical Catalogues.From this documentation it is possible to generate f77 program to load files into arrays or line by line

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